Monte Carlo ray-tracing shows quasilinear scattering coefficients for solar radio waves are accurate for weak scattering but deviate in strong scattering, requiring a speed-based correction in 3D.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
A Monte Carlo simulation on the scattering coefficients of solar radio wave propagation
Monte Carlo ray-tracing shows quasilinear scattering coefficients for solar radio waves are accurate for weak scattering but deviate in strong scattering, requiring a speed-based correction in 3D.